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相关论文: Constraining MeV to 10 GeV majoron by Big Bang Nuc…

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We consider the cosmological effects of sterile neutrinos with the masses of $150- 450$ MeV. The decay of sterile neutrinos changes the thermal history of the Universe and affects the energy density of radiation at the recombination and the…

高能物理 - 唯象学 · 物理学 2020-10-13 Graciela B. Gelmini , Masahiro Kawasaki , Alexander Kusenko , Kai Murai , Volodymyr Takhistov

We show that the predicted primordial helium production is significantly reduced when new measurements of the neutron lifetime and the implied enhancement in the weak reaction rates are included in big-bang nucleosynthesis. Therefore, even…

天体物理学 · 物理学 2009-11-10 G. J. Mathews , T. Kajino , T. Shima

Big-bang nucleosynthesis (BBN) probes the cosmic mass-energy density at temperatures $\sim 10$ MeV to $\sim 100$ keV. Here, we consider the effect of a cosmic matter-like species that is non-relativistic and pressureless during BBN. Such a…

宇宙学与河外天体物理 · 物理学 2024-01-18 Tsung-Han Yeh , Keith A. Olive , Brian D. Fields

Current precision big bang nucleosynthesis (BBN) studies motivate us to revisit the neutron lifespan in the plasma medium of the early universe. The mechanism we explore is the Fermi-blocking of decay electrons and neutrinos by plasma. As…

核理论 · 物理学 2018-05-18 Cheng Tao Yang , Jeremiah Birrell , Johann Rafelski

A cosmological model with a time-varying mass of electrons seems a promising solution for the so-called Hubble tension. We examine the big bang nucleosynthesis (BBN) constraints on the time-varying electron mass model, because a larger…

宇宙学与河外天体物理 · 物理学 2023-05-01 Osamu Seto , Yo Toda

We investigate how the resonant conversion at a temperature $\bar{T}=25$-$65$ keV of a fraction of the CMB photons into an axion-like majoron affects BBN. The scenario, that assumes the presence of a primordial magnetic field and the…

高能物理 - 唯象学 · 物理学 2023-11-20 Antonio J. Cuesta , José I. Illana , Manuel Masip

We explore the effect of neutron lifetime and its uncertainty on standard big-bang nucleosynthesis (BBN). BBN describes the cosmic production of the light nuclides $^1{\rm H}$, ${\rm D}$, $^3{\rm H}$+$^3{\rm He}$, $^4{\rm He}$, and $^7{\rm…

宇宙学与河外天体物理 · 物理学 2023-03-08 Tsung-Han Yeh , Keith A. Olive , Brian D. Fields

Comparing Big Bang Nucleosynthesis predictions with the light element abundances inferred from observational data, we can obtain the strong constraints on some neutrino properties, e.g. number of neutrino species, mass, lifetime. Recently…

天体物理学 · 物理学 2016-08-30 M. Kawasaki , K. Kohri , Katsuhiko Sato

We review the recent proposal by Lattanzi & Valle of the majoron as a suitable warm dark matter candidate. The majoron is the Goldstone boson associated to the spontaneous breaking of ungauged lepton number, one of the mechanisms proposed…

天体物理学 · 物理学 2011-08-04 Massimiliano Lattanzi

In this paper we consider the effects on big bang nucleosynthesis (BBN) of the hadronic decay of a long-lived massive particle. If high-energy hadrons are emitted near the BBN epoch ($t \sim 10^{-2}$ -- $10^2 \sec$), they extraordinarily…

天体物理学 · 物理学 2009-11-06 K. Kohri

We study effects of long-lived massive particles, which decay during the big-bang nucleosynthesis (BBN) epoch, on the primordial abundances of light elements. Compared to the previous studies, (i) the reaction rates of the standard BBN…

高能物理 - 唯象学 · 物理学 2018-12-04 Masahiro Kawasaki , Kazunori Kohri , Takeo Moroi , Yoshitaro Takaesu

We investigate the impact of a nonstandard electron mass $m_e$ on early-Universe thermal history, focusing on neutrino decoupling and Big Bang Nucleosynthesis (BBN). In the standard cosmology, neutrino--electron interactions keep neutrinos…

高能物理 - 唯象学 · 物理学 2026-05-28 Michela Garramone , Stefano Gariazzo , Nicolao Fornengo

During big bang nucleosynthesis, any injection of extra neutrons around the time of the $^7$Be formation, i.e. at a temperature of order $T \simeq 50$~keV, can reduce the predicted freeze-out amount of $^7$Be + $^7$Li that otherwise remains…

高能物理 - 唯象学 · 物理学 2014-10-29 Alain Coc , Maxim Pospelov , Jean-Philippe Uzan , Elisabeth Vangioni

We study Big Bang Nucleosynthesis (BBN) constraints on heavy QCD axions. BBN offers a powerful probe of new physics that modifies the neutron-to-proton ratio during the process, thanks to the precisely measured primordial Helium-4…

高能物理 - 唯象学 · 物理学 2026-03-11 Tae Hyun Jung , Takemichi Okui , Kohsaku Tobioka , Jiabao Wang

Within the first 20 minutes of the evolution of the hot, dense, early Universe, astrophysically interesting abundances of deuterium, helium-3, helium-4, and lithium-7 were synthesized by the cosmic nuclear reactor. The primordial abundances…

天体物理学 · 物理学 2007-05-23 Gary Steigman

Heavy Neutral Leptons (HNLs) are strongly motivated by theory due to their capability of simultaneously explaining the observed phenomena of dark matter, neutrino oscillations and the baryon asymmetry of the Universe. The existence of such…

高能物理 - 唯象学 · 物理学 2020-12-09 Nashwan Sabti , Andrii Magalich , Anastasiia Filimonova

We study the big-bang nucleosynthesis (BBN) with the long-lived exotic particle, called X. If the lifetime of X is longer than \sim 0.1 sec, its decay may cause non-thermal nuclear reactions during or after the BBN, altering the predictions…

天体物理学 · 物理学 2009-11-10 Masahiro Kawasaki , Kazunori Kohri , Takeo Moroi

Big Bang Nucleosynthesis can provide, via constraints on the expansion rate at that time, limits on possible variations in Newton's Constant, $G$. The original analyses were performed before an independent measurement of the…

天体物理学 · 物理学 2009-11-10 Craig J. Copi , Adam N. Davis , Lawrence M. Krauss

We study the impact of light GeV-scale heavy neutral leptons (HNLs) on Big Bang nucleosynthesis (BBN) in the neutrino-extended Standard Model Effective Field Theory ($\nu$SMEFT). We show that, based on very general considerations, BBN…

高能物理 - 唯象学 · 物理学 2026-02-16 Pieter Braat , Jordy de Vries , Jelle Groot , Julian Y. Günther , Juraj Klarić

We investigate Big Bang nucleosynthesis (hereafter, BBN) in a cosmic environment characterized by a distribution of small-scale matter/antimatter domains. Production of antimatter domains in a baryo-asymmetric universe is predicted in some…

天体物理学 · 物理学 2009-10-30 Jan B. Rehm , Karsten Jedamzik
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